Optical Characterization of the SPT-3G Focal Plane

Kavli Affiliate: Keith Thompson | First 5 Authors: Zhaodi Pan, Peter Ade, Zeeshan Ahmed, Anderson Adam, Jason Austermann | Summary: The third-generation South Pole Telescope camera is designed to measure the cosmic microwave background across three frequency bands (95, 150 and 220 GHz) with ~16,000 transition-edge sensor (TES) bolometers. Each multichroic pixel on a detector […]


Continue.. Optical Characterization of the SPT-3G Focal Plane

Optical Characterization of the SPT-3G Focal Plane

Kavli Affiliate: Keith Thompson | First 5 Authors: Zhaodi Pan, Peter Ade, Zeeshan Ahmed, Anderson Adam, Jason Austermann | Summary: The third-generation South Pole Telescope camera is designed to measure the cosmic microwave background across three frequency bands (95, 150 and 220 GHz) with ~16,000 transition-edge sensor (TES) bolometers. Each multichroic pixel on a detector […]


Continue.. Optical Characterization of the SPT-3G Focal Plane

Optical Characterization of the SPT-3G Focal Plane

Kavli Affiliate: John Carlstrom | First 5 Authors: Zhaodi Pan, Peter Ade, Zeeshan Ahmed, Anderson Adam, Jason Austermann | Summary: The third-generation South Pole Telescope camera is designed to measure the cosmic microwave background across three frequency bands (95, 150 and 220 GHz) with ~16,000 transition-edge sensor (TES) bolometers. Each multichroic pixel on a detector […]


Continue.. Optical Characterization of the SPT-3G Focal Plane